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The '-Home College Series'' will contain one hundred short papers on 
a wide range of subjects — biographical, historical, scientilic, literary, domes- 
tic, political, and religious. Indeed, the religious tone will characterize all 
of them. They are written for every body — for all whose leisure is limited, 
but who desire to use the minutes for the enrichment of life. 

These papers contain seeds from the best gardens in all the world of 
human knowledge, and if dropped wisely into good soil, will bung forth 
harvests of beauty and value. 

They are for the young — especially for young people (and older people, 
too.) who are out of the schools, who are full of "business" and "fares," 
who are in danger of reading nothing, or of reading a sensational literature, 
that is worse than nothing. 

One of these papers a week read over and over, thought and talked about 
at "odd tinses," will give in one year a vast fund of information, an intel- 
lectual quickening, worth even more than the mere knowledge acquired a 
taste for solid reading, many hours of simple and wholesome pleasure, and 
ability to talk intelligently and helpfully to one's friends. 

Pastors may organize "Home College" classes, or "Lyceum Beading 
Unions," or "Chautauqua Literary and Scientific Circles," and help the 
young people to read and think and talk and live to worthier purpose. 

A young man may have his own little " college-," all by himself, read this 
series of tracts one after the other, ^there will soon be one hundred of them 
ready.) examine himself on them by the "Thought-Outline to Help the Mem- 
ory," and thus gain knowledge, and, what is better, a love of knowledge. 

And what a young man may do in this respect, a yonng woman, and both 

old men and old women, may do. 

*l J. H. Vincent. 

New Yoke, Jan., 1883. 


Copyright, 18S3, by Phillips & Hunt, New York. 

IJonu College ftumkr Jfiftmi. 


We may reasonably suppose the science of astronomy to 
have originated in the study of the moon. The sun, by its 
superior and unvarying brilliancy, would first attract and 
then baffle the attention of men. The lunar orb, perpetually 
changing, would, because of this peculiarity, become the 
subject of later and more constant observations. Man, even 
as a savage, must have been impressed by " the moon walk- 
ing in brightness " and silently marching in stately grandeur 
among the stars ; while her awesome changes of place and 
form inspired devout feelings, and led him to render divine 
honors to the Queen of Night. She soon came to be 
regarded as the emblem of change. Perhaps it was because 
of her regular irregularity that all lovers have sworn by 
her constancy, though only part of them have kept their 

In very early ages her comparatively rapid motion, in a 
circuit around the earth, afforded a convenient measure of 
time. Her contributions to modern exact astronomy are of 
the highest importance. It is probable that without her aid 
the law of gravitation would never have been discovered. Of 
all the heavenly bodies she is much the nearest and, conse- 
quently, the best known as to surface, configuration, and 
physical peculiarities. 

I. The Moon as a Planet. 

The moon's remarkable proximity is only comparative. 
Her mean distance from the center of the earth is about 
240,000 miles. The use of the telescope, apparently, greatly 
lessened this distance. It is said Sir William Herschel em- 
ployed a telescope of such great power that the moon seemed 


to be within a distance of 40 miles. It is doubtful if a mag- 
nifying power of more than 1,000 can be practically available 
for astronomical purposes. 

Sometimes the moon appears smaller and sometimes larger 
than usual. This can be explained. The moon, 
size a of ar the in her elliptical orbit, answering to the attract- 
ive force of the sun, varies in the course of each 
monthly revolution from ten to twenty thousand miles on 
each side of her mean distance from the earth. This causes a 
corresponding variation in her apparent size. Again, the 
moon appears smaller at the zenith, though actually 4,000 
miles nearer the observer than when at the horizon. This is 
a pure illusion, arising from the instinctive habits of the 
eye in judging distance and magnitude by intervening ob- 
jects. Again, we are deceived by the brightness of the 

This fact dawns upon us when we see the crescent of the 
new moon, as part of a much larger sphere than the old 
moon, which it has been said, time out of mind, to " hold in 
its arms." Thus it appears the moon's disk covers a much 
larger space, in observation and calculation, than it would if 
it were not so bright. This effect of irradiation, as it is called, 
must be allowed for in exact measurements of the moon's 
diameter. The apparent size or angular diameter of the moon 
, a . is about thirty-one minutes. To ascertain the real 

The real ch- * . 

mensions of diameter of the moon, we construct an imaginary 

the moon. . . -,-,.-, i -.. -, i- • 

right-angled triangle, whose perpendicular line is 
the known distance of the moon from the earth, and its base 
line half the angular diameter. From this we find it to be a 
little over one quarter of that of the earth, or about 2,160 
miles. The surface of the earth contains about 196,870,000 
square miles. The actual surface of the moon is rather more 
than two twenty-ninths of the earth's surface, and, therefore, is 
almost exactly equal to the areas of North and South Amer- 
ica, exclusive of their islands. The earth is more dense than 


the moon; so that, while in volume or bulk our planet is fifty 
times larger, her mass is eighty times greater than that of 
her satellite. With the naked eye large dusky patches are 
visible on the moon, a frequent observation of . . , 

m 1 . Axial and or- 

which leads to the conclusion that the same hemi- Mtai motions 

. . of the moon. 

sphere is always turned to the earth. Obviously, 
the moon makes one revolution on her axis in the same time 
that she revolves around the earth, and thus always presents 
the same side to us. However, a small part of this, as well 
as a small part of the other, side slowly swings in and out of 
view. The following may throw light upon this balancing 
motion or " apparent rocking to and fro " of the globe of the 
moon. The moon's rotation on her axis does not exactly co- 
incide with her revolutionary motion at every point of her 
orbit around the earth. As a matter of fact, when the moon 
is approaching perigee, or nearest the earth, her orbital motion 
is accelerated; and when approaching apogee, or farthest 
from the earth, it is retarded. " Her axial motion is uniform, 
while her orbital motion is not." In proportion to the dif- 
ference between the orbital motion and the axial motion can 
we see alternately a little farther around on the eastern and 
western limbs of the moon. This alternation is called libra- 
tion in longitude. Certain regions on the northern and 
southern limbs of the moon, also, alternately recede from 
sight and come into view. This is called libration in lati- 
tude, and is due to the fact that the axis of the moon is not 
quite perpendicular to the plane of her orbit; the poles of 
the moon being turned six degrees and a half alternately 
toward and from the earth. A kindred phenomenon to li- 
bration in longitude is called diurnal libration, since it occurs 
daily, and parallactic libration, since it is due to the point 
from which the moon is viewed; whether from the zenith, or 
eastern or western horizon, or any intermediate point. By 
these three librations two-elevenths of the moon's surface is 
swayed out of and into view; six tenths may be seen at one 


time or another, while the remaining four tenths are forever 
concealed from view. In accounting for these phenomena 
of the moon, we commence with her ellipsoidal form and el- 
liptical orbit of slight eccentricity. The plane of this orbit 
is inclined to the ecliptic by an angle of about five degrees. 
The ecliptic is the circle described by the sun in its apparent 
motion around the heavens. The two points where the 
moon's orbit cuts this circle are called her nodes. These 
have a westward motion, and complete the circuit of the ec- 
liptic in about nineteen years. The moon revolves around 
the earth from west to east. Moving at the rate of about 
twelve degrees a day, she completes the circuit of the 
heavens in about thirty days. 

The moon, revolving in her orbit, comes into different posi- 
The phases, as- tions with reference to the earth and the sun. 
nods 5 ' o? d the These different positions are called the aspects of 
moon. ^g moon# The moon is a dark opaque globe ; but 

the half that is toward the sun is always bright from borrowed 
light. The different portions of this illumined half, as they are 
turned toward the earth, constitute the phases of the moon. 
"When the moon is in the same part of the heavens as the 
sun, or rather is between the earth and the sun, the aspect is 
that of "conjunction; " and, as the darkened side is toward 
the earth, the phase is a new moon, a corruption of " no 
moon." Where the phase of the moon is crescentic, with the 
convex side toward the sun and its horns toward the east, it 
is called " first quarter," and when with its horns turned to- 
ward the west it is called " last quarter." From the first 
quarter to the last quarter we may note the following as- 
pects and phases. When the moon appears ninety degrees, 
away from the sun, the aspect is at " quadrature," and the 
phase is that of a "half moon;" when past quadrature, the 
bright side appears as a " three-quarter moon " and is called 
" gibbous; " when the moon is in the opposite part of the heav- 
ens to the sun, the aspect is that of " opposition," and the 


phase is that of the " full moon." The moon has two periods 
of unequal length, the sidereal and synodical. In making 
a complete revolution around the earth, the moon appears to 
pass around from a star to the same star again. The period 
of time required for this is about twenty-seven and one third 
days, and may be called, the sidereal month. But, to pass 
from one aspect around to the same aspect again, while the 
earth is moving forward in its orbit, the moon must make 
more than a complete revolution. This occupies a period of 
about twenty-nine and one half days, and may be called 
the synodical month. Owing to the moon's east- 

/ L . , ° -^ . The retarda- 

ward motion, she rises, on an average, fifty mm- tion of the 
utes later each day. If the moon was on the horizon 
at a certain hour to-day, she would be twelve degrees below 
the horizon at the same hour to-morrow; having traveled 
thirteen degrees in the meantime, or twelve degrees faster 
than the sun appears to move. The moon's latitude, nearness 
to the earth, and position in her orbit with reference to the 
equinoxes, effect more or less of a variation in this daily re- 
tardation. This is not likely to attract attention unless it 
occurs during full moon. The longest retardations for full 
moon occur in the spring, the greatest being in March. The 
least retardations for full moon occur in the months of Au- 
gust, September, and October, the least of all being in Sep- 
tember. The " harvest moon " is the full moon of September, 
and the " hunter's moon " is the full moon of October. 

II. The Moon as a Satellite. 

Correctly speaking, the earth and moon are a pair of 
planets revolving around a common center of gravity. This 
common center, owing to the earth's greater size and weight, 
is located within it, at a distance of two thousand miles from 
that part of its surface which, happens to be turned toward 
the moon. And in addition to this motion the moon, no less 
truly than the earth, revolves around the sun, whose attrac- 


tion for each one of these planets is nearly the same in de- 
gree. Because of this, and their mutual attraction, the sun 
does not force them apart — they are traveling companions. 
Our planet, greater in size, has the stronger attracting power, 
yet enjoys the moon's beneficent ministrations ; and hence 
the common expression, " The earth and her satellite." The 
analysis of the phases and aspects of our satellite, or pecul- 
iarities of lunar motion, has been. carried to an almost un- 
hoped-for degree of perfection by the most skillful ob- 
servers and most acute mathematicians. Observation and 
calculation have been pushed to an equal point of delicacy 
to detect the exact proportion of the moon's influence, among 
The tides and others, in producing the tides, but without equally 
the moon. satisfactory results. The whole philosophy of 
tides has not yet been constructed. But there are certain 
very interesting facts which have been made apparent. The 
most ancient nations living near the ocean could not fail to 
have noticed the alternate rise and fall of the surface of 
the sea twice in the course of twenty-four hours and fifty- 
one minutes. They must also have observed the singular 
coincidence with this of the diurnal motion of the moon. 
The whole matter, however, remained enveloped in mystery, 
until the discovery of the law of gravitation made an expla- 
nation possible. The moon is now known to be the cause of 
the tides. In so far as the moon is responsible for the tides, 
they are due to her varying power of attraction. The moon 
is but thousands, while the sun is millions, of miles distant. 
Hence, as the power of attraction decreases as the square of 
the distance increases, it may be readily seen why the tides 
are the more largely controlled by the moon. Notwithstand- 
ing the sun's great distance from the earth, his attractive in- 
fluence upon the tides is about four tenths as great as that 
of the moon, or as two to five* The earth produces a centrif- 
ugal — or center-fleeing — force by revolving about a com- 
mon center of gravity. Hence it becomes depressed at the 


polar, and protuberant at the equatorial, regions. Thus of 
itself the earth contributes somewhat to the height of the 
tides by a kind of swinging off of the waters on that side 
farthest from the moon. We cannot precisely determine all 
the influences and their exact mode of interaction in pro- 
ducing tidal peculiarities. They are almost innumerable, 
and doubtless some of them elude detection. Others are 
known, such as the varying distance of the moon from the 
earth ; its position, north, south, or at the equator ; the va- 
rying distance of the earth from the sun; the direction and 
peculiar conformity of shore lines, and the meeting of tidal 
waves. These last two are found in conjunction in the Bay 
of Fundy, where the water rises to the unusual height of 
sixty and seventy feet. "At small islands in mid-ocean the 
tides never rise to a great height, sometimes even less than 
one foot ; and the average height of the tides for the islands 
of the Atlantic and Pacific Oceans is only three feet and a 
half," while the average along the continental coast-lines is 
v not less than four or five feet. The sea is at flood-tide when 
it is rising, and at ebb-tide when it is falling. When at its 
greatest height it is high water, and when lowest it is low 
water. At new moon, the sun and moon being on the same 
side of the earth, or in " conjunction," unite their forces, and 
we have the greatest ebb and flow, called the spring-tides. 
Their influences antagonize each other when the moon is in 
her first or third quarter, and we have neap, or low tides. 
We have the spring-tide, also, when the moon is in " oppo- 
sition." Hence we have two spring-tides and two neap-tides 
occurring each month. Owing to the disposition of the wa- 
ters to remain at rest, the moon's influence is not immediately 
felt; so that high tide occurs about three hours after the 
moon has passed over or beyond that point. In producing 
high tides at the points immediately under it, the moon 
draws the waters from the sides of the earth distant one 
fourth of its circumference, where of necessity there will be 


low tides. But on the opposite side of the earth from the 
moon there will also be high tides. 

"In one case, as the tide nearest the moon, the water is 
drawn from the earth; in the other, as the side farthest from 
it, the earth is drawn from the water." The chief cause of 
this is the moon's differing attractive influence on the near 
and farther side of our planet. 

How strikingly the wisdom, power, and beneficence of 
Him " who hath measured the waters in the hollow of his 
hand " is illustrated in the tidal movements and their results ! 
If the moon does not supply, at least it liberates and sets in 
motion tidal energy of a character most astonishing and be- 
neficent to the world. From a practical point of view, the 
work done by the tides is of unspeakable importance. For 
six hours the world of waters surges simultaneously, in one 
resistless wave, to the east; and, after remaining at rest for 
a few moments, rushes back in one great tidal current to the 
west. This is continually repeated. By this ceaseless agi- 
tation the great body of waters, otherwise putrid and a store- 
house of pestilential vapors, is kept pure, and also purifies 
the atmosphere. The beautiful white-crested waves cleanse 
the wind of its impurities, and send it back to the land more 
fit for the use of man. " The sea washes every shore, puri- 
fies every cove, bay, and river twice every twenty-four 
hours." Impurities are carried far from the shore and sunk 
into the depths of the never- stagnant sea. Great tidal waves 
rush up rivers and render such of these as are more shallow 
navigable, and thus facilitate the purposes of commerce. 
The flow and ebb of the tide transports heavy merchandise, 
which, if done by artificial means, would cost the city of Lon- 
don alone, thousands, and perhaps millions, of pounds yearly. 
One hundred years ago, the same city was supplied with 
water by pumps worked by tidal mills at London Bridge. 
By the aid of tidal mills the rise and fall of the water can 
be converted into any form of mechanical power. We do 


not utilize the tides to the extent of their capacity. It re- 
mains for the future to develop this comparatively hitherto 
un worked power. 

How wonderful that the moon, who is so remote, can 
perform for us so many important offices ! Over Ideas of the 
the great distance of 240,000 miles she reaches m(,on,s influ : 

o 7 ence upon and 

out an invisible hand ; and with its ever-open relation to our 

1 -it world. 

palm, through tidal forces and borrowed light, she 
ministers to the well-being of our world and its inhabitants. 
The superstitious notions of the moon's influence upon the 
weather, animals, plants, and food prepared at its particular 
phases, are wholly unsupported by philosophy or fact. But 
that " He hath appointed the moon for seasons," as also its 
beneficent disturbing influence upon the waters of the vast 
oceans, are matters of both philosophy and fact. How dis- 
astrous to the world would be the loss of its tidal energy ! How 
much of human happiness is due to the presence of our 
beautiful lunar orb ! How cheerless would be our long 
winter evenings if she was to disappear forever from our 
night-draped sky ! Such a disappearance is highly improb- 
able, at least so long as mankind needs her service. If the 
cometic origin of the moon be true, she may be lost to us, 
by some larger body than the earth passing near and carry- 
ing off our Empress of Night. Or at some day the earth 
may arrest and detain in his giant grasp another comet as a 
revolving satellite, and thus have two or even more moons, 
as is the case with some of the other planets. A more 
probable theory of the moon's origin is, that about the time 
that our globe, from thin nebulous matter diffused through 
space, condensed into its present shape, its satellite was 
formed in the same way, from fragments thrown off by the 
planetary mass. Hence the probability that the moon is 
composed of materials such as constitute our globe, and is 
of itself a dark body, shining only by reflected light. 


III. The Moon as a World. 
The early Chaldean astronomers held that the moon was a 

Emiy notions g ioDe > on ^ half of which was made of fire, and 
conSitu h t?o C 2! wnicn > D y revolving upon its axis, presented its 
etc. different sides in succession. This hypothesis 

was exploded when it was discovered that the bright portion 
of the moon is always that which is turned at once to the 
sun and to the earth. The theory which obtained about 640 
B. C, that a portion of the moon's light is inherent, because 
of a dim globular light observed resting in the crescent or 
bowl of the moon, has since then been attributed to its true 
cause — the reflected light of the earth. Some of the Pythag- 
orean philosophers taught that the moon is totally unlike 
the earth, and regarding her as a smooth crystalline body 
reflecting light as a mirror, they supposed the spots on her 
Early notions disk to be the reflection of the oceans and con- 
configuratio ?, tinents of our earth. Others have recognized in 
etc - these spots the configuration of a human form. 

A French superstition that lingers to the present day holds 
this to be the image of Judas Iscariot, transported there for 
the betrayal of his Master. These spots bear a quaint re- 
semblance to a human face. This idea is more than a nurs- 
ery tradition, it is of the most A^enerable antiquity ; but 
with the ancients the " man in the moon " is of the softer 
sex. We find in Plutarch a quotation from an early Greek 
poet which has received this translation : 

"Over the orb shines a resplendent light. 
In the midst of which a damsel's face is seen, 

Whose cheeks suffused display her blushes bright ; 
Her eye cerulean, or a pale sea green." 

While fancy makes pictures of these unchangeable spots, 
and weaves them into poetic conceits, science, 

eiatSns P of r t e he seeking their true explanation, reveals wonders 
surpassing those of pure imagination. The first 

users of the telescope supposed, from these spots appearing 

THE 310 ON. 11 

smooth as water, that they were vast seas, and accordingly 
gave to them appropriate Latin names. But higher tele- 
scopic power showed these regions to have more or less of 
an uneven surface with permanent elevations and depressions, 
and thereby caused men to abandon the sea theory. These 
spots or plains, however, are comparatively smooth, because 
of the greater irregularities of the other portions of the 
moon's surface, Instead of regular mountain ranges and 
undulation of hill and valley, we find the surface of the 
moon differs from that of the earth, in having but few 
mountain ranges, there being a prevalence of crater-like 
irregularities and a general tendency to circular shape, as 
seen in its numerous ring-shaped mountains and plains. 
These plains or depressions are the dark spots seen upon the 
lunar disk ; some of which sink lower than 4,000 feet below 
the general surface. "In consequence of the small gravita- 
tion of the moon, utter absence of the expansive power of 
ice shivering the cliffs, or the leveling power of rains, prec- 
ipices can stand in perpendicularity, mountains shoot up like 
needles, and cavities three miles deep remain unfilled." Many 
of the crater-like mountains, with a diameter of more than 
fifty miles, have rings within rings. Often mountains of 
immense height are seen in these craters, mountains within 
mountains, seemingly constructed of volcanic matter, from 
former eruptions. These mountains vary greatly in size ; 
some being so small that they can scarcely be detected with 
the most powerful telescope, aud others again so large as to 
bear a sensible proportion to the moon's diameter. Its 
loftiest mountain, Doerfel, is 24,945 feet high. Our monarch 
of mountains, Mont Blanc, is surpassed in height by no less 
than 28 different mountains of the moon. The wonderful 
feat of measuring the lunar mountains is accomplished by 
ascertaining the time of revolution and observing the change 
of illumination ; the daylight struggling with the dark 
alons^ the terminator — the line of the moon's sunrise or sun- 


set. In consequence of the slow rotation of the moon on its 
Day and night ax i s > i ts day and night must "be each 304 hours 
on the moon. \ 0Yi g^ or twenty-nine and a half times as long as 
ours. Each season consists of but three days and three 
nights, and twelve days and nights constitute a year of the 
same length as ours. For fifteen days the sun shines unin- 
termittingly, rendering the lunar day more scorching than 
the fiery breath of the sirocco. For fifteen nights dark- 
ness and intense cold succeed the moon's day. "And 
thus each of its long days will be in reality a summer 
and every night a winter — the morning twilight spring and 
the evening twilight autumn." Only on the moon there is 
no twilight, since it has no water to produce vapor, and the 
closest scrutiny fails to detect an atmosphere. Because of 
the atmosphere of our planet we see the image of a heavenly 
body a short time before it appears above, as also a short 
time after it disappears below, the horizon. But, instead of 
the same phenomenon, when the moon passes over stars they 
instantly disappear, and their reappearance is as sudden. 

From this and other phenomena, which need not here be 
isthemoonin- considered, we may reasonably infer the absence 
habited? on t ] ie moon of all forms of life, resembling those 

with which we are familiar on the earth. In an early age 
the belief found favor that the moon was an inhabited world, 
like the earth. Some, taking into consideration the length of 
the lunar day and night, have thought the moon, if inhab- 
ited, must be by creatures fifteen times as large as terrestrial 
beings, and with architectural achievements correspondingly 
great. Others, again, upon the discovery of the absence of 
favorable conditions for life upon this side, have asserted the 
existence of these conditions upon the opposite side of the 
moon. The reasoning for this is now confessedly falla- 
cious. Even with an atmosphere on the moon, there would 
be great difficulty in supporting life with any degree of com- 
fort. Indeed, it would not be at all possible only under very 


peculiar circumstances. The moon has a very narrow tem- 
perate zone on the margin of its two hemispheres; but it is 
perpetually changing because of the moon's eccentric mo- 
tions. To live on the moon is to keep in this zone. To do 
this, the lunarians, birds, beasts, reptiles, and insects, must 
be constantly on the move; at the rate of ten miles an hour 
in a sort of " Noah's Ark " procession. 

Many believe that the moon has not always been water- 
less and airless: but find difficulty in explaining Physical condi- 

* J r & tion of the 

the processes by which she reached her present moon. 
condition. However, the opinion generally entertained is, 
that, as the moon's interior cooled, the water and air became 
soaked up in the porous lava of its substance. There are 
marked signs of former great volcanic activity on the moon; 
but it seems to have reached a burnt-out and chilled phase of 
existence many ages ago. The selenography and especially 
the mapping of the moon has reached such a point of perfec- 
tion, that the least change in its surface, recognizable from 
the earth, could not escape notice. No change, in the visible 
configuration of the moon, has as yet been detected ; and the 
supposition is that long ago it arrived at a terminal condi. 
tion. Indeed, some are even disposed to say, " In the survey 
of its wonderful features, even in the smallest details, we are 
presented with the sight of objects of such transcendent 
antiquity, as to render the oldest geological features of the 
earth modern in comparison." It is quite probable as the 
moon looks to-day so will it appear to observers thousands 
of years hence. An ideal view of the moon-world and its 
phenomena may be pleasing and profitable. We A visit t0 the 
pass no planets or stars in our journey to the wiTali-htof 
moon; for it is the nearest of the larger heavenly its phenomena. 
bodies. In imagination we traverse the 240,000 miles of 
space and stand at sunrise upon one of the mountain tops of 
the moon. Over head is a cloudless sky, of inky blackness; 
the background of countless brilliant stars, and of the earth, 

14 THE MO OX. 

which is in appearance equal to many moons, and, when 
passing between the sun and the moon, is like a dark sphere in 
a circle of glittering gold and rubies. From the dark horizon, 
the sun suddenly darts 'his dazzling beams upon the tops 
of the mountains; yet for a time leaving the flanks and val- 
leys still wrapped in total night. In the absence of air and 
vapor there is no gradual transition of night into day; no 
penciling streaks, no gilding and glowing, which make 
earth's sunrise so beautiful; yet there is increase of illumina- 
tion as more and more of the sun's disk becomes visible 
above the horizon. The light, with a motion twenty-eight 
times slower than upon the earth, creeps down the mountain 
side, across the plain, and into the fearful blackness of the 
yawning crater. 

Look where we may, we see vast regions of the wildest 
volcanic desolation, in which the ground is honey-combed Avith 
countless round pits or craters, some of them of immense 
depth and upward of four miles in diameter. On our right 
are steep gorges and precipitous chasms of appalling depth 
and blackness, and on our left cliffs, crags, and peaks tower 
far above us. We gaze upon the debris of long since ex- 
pired volcanoes, but look in vain for a single vestige of past 
or present organic life. " No heaths or mosses soften the 
sharp edges and hard surfaces, no tints of cryptogamous or 
lichenous vegetation give a complexion of life to the hard 
fire-worn countenance of the scene. The whole landscape, 
as far as the eye can reach, is a realization of a fearful dream 
of desolation and lif elessness ; not a dream of death, for that 
implies evidence of pre-existing life, but a vision of a world 
upon which the light of life has never dawned." In the 
midst of this dreary, desolate grandeur we look in vain for 
oceans, lakes, or seas; we listen in vain for the hum of in- 
dustry or the sounds of wind or water, where there is no 
life to break the stillness, no breeze to murmur, " no brook 
to plash, no ocean to boom and foam." Let this desolate, 


craggy, motionless world be filled with the activities of our 
own ; and, in the absence of air, which is the medium of 
communication with the organs of hearing, it would still be 
a realm of dead silence. In vain would lips quiver and 
tongues essay to speak. The r'attle of drums, the crash of 
musketry, the thunder of a thousand cannons would produce 
no sound in that airless world. At the close of the moon's 
long clay we see, in glorious perfection, the red protuber- 
ances, crimson flame billows, corona and zodiacal light of the 
sun; as during the day we may have seen its spots and 
faculse. During the lunar night periods of twenty-four 
hours each can be marked off by the successive reappear- 
ances of certain surface features of our globe. The positions 
of the constellations can be used for a similar purpose. Oc- 
casionally comets are seen in all their glory. The planets 
appear regularly every night; but meteors are never seen. 
Yet meteoric particles, sometimes singly and sometimes in 
showers, frequently smite the face of the moon. They meet 
with no resisting atmosphere, to melt them by its heat or 
break the velocity of their descent. These particles, under 
their initial velocity and the moon's attraction, crush into its 
surface with a force greater than that of a cannon ball 
striking a target. Kepler, though forced to abandon the 
theory after measuring the dimensions of some of the moon's 
craters, at first thought that they were artificial excavations 
in which the inhabitants sheltered themselves during the 
long and scorching days. They would be no less necessary 
as a protection from this bombardment of meteoric particles 
than from the frightful extremes of heat and cold. 



" And God said, Let there be lights in the firmament of 
the heaven to divide the day from the night ; and let them 
be for signs, and for seasons, and for days, and years: and 
let them be for lights in the firmament of the heaven to give 
light upon the earth: and it was so." — Gen. i, 14. 

"The sun to rule by day; the moon and stars to rule by 
night; he appointed the moon for seasons." — David. 

" When I consider thy heavens, the work of thy fingers, 
the moon and the stars, which thou hast ordained; what is 
mat], that thou art mindful of him ? and the son of man, that 
thou visitest him." — David. 

""Who there inhabit must have other powers, 
Juices and veins, and sense and life, than ours ; 
One moment's cold like theirs would pierce the bone, 
Freeze the heart's blood, and turn us all to stone." 

"Some have asked whether the myriads of distant worlds 
were inhabited. It is not known. Perhaps it is a sufficient 
cause of their being that they should testify so effectually of 
God to every man, whether savage or sage, in all ages of 
time." — Henry W. Warren, D.D. 

" The poet's eye, in a fine frenzy rolling, 

Doth glance from heaven to earth, from earth to heaven ; 

And, as imagination bodies forth 

The forms of things unknown, the poet's pen 

Turns them to shapes, and gives to airy nothing 

A local habitation. and a name."— Shakspe are. [ 

the nvioOKr. 

[thought outline to help the memory.] 

1. Value of moon to astronomy ? 

2. Planet. Distance from earth? Apparent size of the moon? How find real 

size? Compare with N. and S. America? How much of moon's surface 
never seen ? Various notions? 

3. Satellite. Power of sun on moon and earth ? Cause of tides ? Remarkable 

tides? Various kinds of tides ? Value? Uses of moon to us? 

4. A World. Theory of Chaldean astronomers? Various notions? Height 

of moon-mountains ? Length of its clay and night ? Its seasons ? Inhab- 
ited ? Theory as to how moon came to be in its present condition? What 
one would see on a visit to the moon ? 

Nn. 1. Biblical Exploration. A Con- 
densed Manual on How to Study the 
Bible. By J. H. Vincent, D.D. Full 
and rich 10 

No. 2. Studies of the Stars. A Pocket 
Guide to the Science of Astronomy. 
By H. W. Warren, D.D 10 

No. 3. Bible Studies for Little People. 
By Eev. B. T. Vincent 10 

No. 4. English Ilistory. Bv J. H. Vin- 
cent, D.D 10 

No. 5. Greek History. By J. II. Vin- 
cent, D.D 10 

No. •<>. Greek Literature. Bv A. D. 
Vail, D.D 20 

No. 7. Meraorinl Days of the Chautau- 
qua Literary and Scientific Circle 10 

No. 8. What Noted Men Think of the 
Bible. By L. T. Townscnd, D.D 10 

N». 9 William Cullen Bryant 10 

No. 10. What is Education? By Wm. 

P. Phelps, A.M 10 

No. 11. Socrates. By Prof. W. P. Phelps, 
A.M 10 

No. 12. Pestalozzi. Bv Prof. W. F. 
Phelps, A.M !.. 10 

No. 13. Anglo-Saxon. By Prof. Albert 
S. Cook. .' 20 

No. 14. Horace Mann. By Prof. Wm. 
F. Phelps, A.M 10 

No. 15. Froebel. Bv Prof. Wm. P. 
Phelps, A.M 10 

No. 16. Roman History. Bv J. H. Vin- 
cent, D.D 10 

No. 17. Roger Ascham and John Sturm. 
Glimpses of Education in the Six- 
teenth Centurv. Bv Prof. Wm. F. 
Phelps, A.M 10 

No. 18. Christian Evidences. By J. H. 
Vincent, D.D 10 


No. 19. The Book of Books. By J. M. 

Freeman, D.D 10 

No. 20. The Chautauqua Hand-Book. 

By J. H. Vincent, D.D 10 

No. 21. American History. By J. L. 

Hurlhut, A.M 10 

No. 22. Biblical Biology. By Rev. J. 

H. Wvthe, A.M., M.D... 10 

No. 2.1. English Literature. By Prof. 

J. H Gilmore 20 

No. 2i. Canadian History. By James 

L. Hughes 10 

No. 25. Self-Education. Bv Joseph Al- 

den, D.D., LL.D 10 

No. 26. The Tabernacle. By Rev. John 

C.TIill 10 

No. 27. Readings from Ancient Classics. 10 
No. 28. Manners and Customs of Bible 

Times. By J. M. Freeman, D.D 10 

No. 29. Man's Antiquity and Language. 

Bv M. S. Terry, D.D 10 

No. 30. The World of Missions. By 

Henry K. Carroll 10 

No. 31. What Noted Men Think of 

Christ. Bv L. T. Townsend, D.D.... 10 
No. 32. A Brief Outline of the History 

of Art. Bv Miss Julia B. De Forest. . 10 
No. 33. Elihu Burritt: "The Learned 

Blacksmith." By Charles Norlhend. 10 
No. 34. Asiatic History : China, Corea, 

Japan. By Rev. Wm. Elliot Griffis. . 10 
No. 35. Outlines of General History. 

By J. If. Vincent, D.D .". 10 

No. 36. Assembly Bible Outlines. By 

J. II. Vincent, D.D 10 

No. 37. Assembly Normal Outlines. By 

J. H. Vincent, D.D 10 

No. 38. The Life of Christ. By Rev. 

J. L. Hurlbut, M.A 10 

No. 39. The Sunday-School Normal 

Class. By J. H. Vincent, D.D 10 

Published by PHILLIPS & HUNT, 805 Broadway, New York.